Results 121 to 130 of about 884 (199)

Crushing of interstellar . . . [PDF]

, 2005
We model the hydrodynamic interaction of a shock wave of an evolved supernova remnant with a small interstellar gas cloud like the ones observed in the Cygnus loop and in the Vela SNR.
F. Reale, R. Rosner, A. Siegel, G. Peres, S. Orlando, F. Bocchino, T. Plewa   +6 more
core  

Structure and Fragmentation Scale of a Massive Star-forming Filament in NGC 6334: High-resolution Mid-infrared Absorption Imaging with JWST

The Astrophysical Journal Letters
Dense filaments are believed to be representative of the initial conditions of star formation in molecular clouds. We have used the MIRI instrument on JWST to image the massive filament NGC 6334M at d  ∼ 1.3 kpc with unprecedented resolution and dynamic ...
Philippe André, Michael Mattern, Doris Arzoumanian, Yoshito Shimajiri, Annie Zavagno, Daisei Abe, Delphine Russeil   +6 more
doaj   +1 more source

⁶⁰Fe deposition during the late Pleistocene and the Holocene echoes past supernova activity. [PDF]

Proc Natl Acad Sci U S A, 2020
Wallner A, Feige J, Fifield LK, Froehlich MB, Golser R, Hotchkis MAC, Koll D, Leckenby G, Martschini M, Merchel S, Panjkov S, Pavetich S, Rugel G, Tims SG.   +13 more
europepmc   +1 more source

Association Reaction of Gaseous C₂H₄ in Femtosecond Laser Filaments Studied by Time-of-Flight Mass Spectrometry. [PDF]

ACS Omega, 2021
Matsuda A, Tani K, Takeuchi Y, Hayakawa Y, Hishikawa A.   +4 more
europepmc   +1 more source

Investigations of MWISP Filaments. I. Filament Identification and Analysis Algorithms, and Source Catalog

The Astrophysical Journal Supplement Series
Filaments play a crucial role in providing the necessary environmental conditions for star formation, actively participating in the process. To facilitate the identification and analysis of filaments, we introduce Directional and Positional Consistency ...
Yu Jiang, Xuepeng Chen, Sheng Zheng, Zhibo Jiang, Zhiwei Chen, Yao Huang, Yang Su, Li Sun, Jian-Cheng Feng, Haoran Feng, Ji Yang   +10 more
doaj   +1 more source

Properties of interstellar filaments as derived from $Herschel$, $Planck$, and molecular line observations

, 2017
Proceedings of the Star Formation in Different Environments, ICISE, Quy Nhon, Vietnam, 2016, (eds. D. Johnstone, T. Hoang, F. Nakamura, Q. Nguyen-Luong, and J. T. Tranh Van)
openaire   +2 more sources

Filamentary Hierarchies and Superbubbles. II. Impact of Superbubbles and Galactic Dynamics on Filament Formation and Fragmentation

The Astrophysical Journal
Large-scale phenomena in spiral galaxies such as shear, supernovae, and magnetic fields all contribute to the formation and subsequent evolution of filamentary structure and star formation within them.
Rachel Pillsworth, Ralph E. Pudritz, Eric W. Koch, Theo J. O’Neill   +3 more
doaj   +1 more source

Probing the Magnetic Fields and Dust Properties in the Young Embedded Star-forming Region AFGL 6366S Using Near-infrared and Optical Linear Polarimetry

The Astrophysical Journal
We present near-infrared (NIR) and optical linear polarimetry toward the partially embedded cluster AFGL 6366S. The polarization ranges from 0.44% to 10.3% in NIR and from 0.16% to 11.22% in the optical bands. The position angle spans 1°−179° in both the
Samrat Biswas, Biman J. Medhi, Motohide Tamura, H.S Das, Jungmi Kwon   +4 more
doaj   +1 more source

Tailoring Vibrational Signature and Functionality of 2D-Ordered Linear-Chain Carbon-Based Nanocarriers for Predictive Performance Enhancement of High-End Energetic Materials. [PDF]

Nanomaterials (Basel), 2022
Lukin A, Gülseren O.
europepmc   +1 more source

Considering light-matter interactions in the Friedmann equations. [PDF]

Proc Math Phys Eng Sci, 2022
Vavryčuk V.
europepmc   +1 more source